Paquette, J.; Fray, N.; Cottin, H.; Engrand, C.; Bardyn, A.; Stenzel, O. J.; Merouane, S.; Hilchenbach, M.; Alexander, C.M.O.; Langevin, Y.: The D/H ratio in cometary dust measured by Rosetta/COSIMA. 49th Lunar and Planetary Science Conference, The Woodlands, Texas, USA (2018)
Merouane, S.; Gunther,, S.; Chitarra, O.; Stenzel, O. J.; Hilchenbach, M.; Engrand, C.; Tarcea, N.: Investigation of Antarctic Micrometeorites and Selected Carbonaceous Chondrites by Raman Sprectoscopy, Electron Microscopy and Mass Spectrometry. 81st Annual Meeting of the Meteoritical Society, Moscow, Russia (2018)
Guenther, S.; Merouane, S.; Hilchenbach, M.; Engrand, C.: Composition of micrometeorites compared to carbonaceous chondrites and comet 67P/Churyumov-Gerasimenko. European Planetary Science Congress 2017, Riga, Latvia (2018)
Nuth, J. A.; Johnson, N. M.; Ferguson, F. T.; Hilchenbach, M.; Merouane, S.; Paquette, J. A.; Stenzel, O.; Cottin, H.; Fray, N.; Bardyn, A.et al.; Baklouti, D.; Le Roy, L.: Refractory Organics in Comet 67P/Churyumov-Gerasimenko: Additional Evidence for Large-Scale Mixing in the Primitive Solar Nebula? 48th Lunar and Planetary Science Conference, The Woodlands, Texas (2017)
Bardyn, A.; Baklouti, D.; Briois, C.; Cottin, H.; Fray, N.; Engrand, C.; Fischer, H.; Hilchenbach, M.; Merouane, S.; Modica, P.et al.; Paquette, J.; Ryno, J.; Silén, J.; Stenzel, O.; Thirkell, L.: Cometary dust composition and its variation as seen by COSIMA over nearly two years of the Rosetta mission. Symposium Comets - A new vision after Rosetta and Philae, Toulouse, France (2016)
Langevin, Y.; Hilchenbach, M.; Ligier, N.; Merouane, S.; Hornung, K.; the Team Cosima: Evolution of the typology of cometary particles collected by the COSIMA instrument from before to after perihelion. EGU General Assembly, Vienna, Austria (2016)
Langevin, Y.; Hilchenbach, M.; Ligier, N.; Merouane, S.; Hornung, K.; Vincendon, M.; Engrand, C.; Schulz, R.; Kissel, J.; Rynö, J.et al.; the COSIMA Team: Typology of cometary particles collected by COSIMA during the orbital phase of Rosetta (August 2014 September 2016). Symposium Comets - A new vision after Rosetta and Philae, Toulouse, France (2016)
Merouane, S.: Evolution of the Dust Particles Size Distribution and Flux from Comet 67P around Perihelion Measured by the COSIMA Instrument on-board Rosetta. 50th ESLAB Symposium: From Giotto to Rosetta, Leiden, Netherlands (2016)
Hilchenbach, M.; Hornung, K.; Kissel, J.; Langevin, Y.; Merouane, S.; The COSIMA Team: Mechanical properties of cometary dust particles as observed in the inner coma of 67P/Churyumov-Gerasimenko. IAU General Assembly Meeting, Honolulu, USA (2015)
How does our star heat its outer atmosphere, the solar corona, to unimaginable temperatures of up to 10 million degrees Celsius? With unprecedented observational data from ESA's Solar Orbiter spacecraft and powerful computer simulations, ERC starting grant awardee Pradeep Chitta intends to bring new momentum to the search for the coronal heating mechanism.
The research group “Solar Lower Atmosphere and Magnetism” (SLAM) studies the conditions and dynamic processes in the atmospheric layer between the solar surface (photosphere) and the overlying chromosphere, an approximately 2000 km thick gas layer.
The main research fields of the department "Sun and Heliosphere" are covered by the research groups "Solar and Stellar Coronae", "Solar Lower Atmosphere and Magnetism", "Solar and Stellar Magnetohydrodynamics" and "Solar Variability and Climate".